Morphology Study for GeV Emission of the Nearby Supernova Remnant G332.5-5.6

Morphology Study for GeV Emission of the Nearby Supernova Remnant G332.5-5.6

Spatial template is important to study the nearby supernova remnant (SNR). For SNR G332.5-5.6, we report a gaussian disk with radius of about 1.06 degrees to be a potential good spatial model in the gamma-ray band. Employing this new gaussian disk, its GeV lightcurve shows a significant variability...

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Veröffentlicht in:arXiv.org 2024-03
Hauptverfasser: Ming-Hong, Luo, Qing-Wen Tang, Xiu-Rong Mo
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Emission analysis
Gamma rays
Supernova remnants
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description Spatial template is important to study the nearby supernova remnant (SNR). For SNR G332.5-5.6, we report a gaussian disk with radius of about 1.06 degrees to be a potential good spatial model in the gamma-ray band. Employing this new gaussian disk, its GeV lightcurve shows a significant variability of about 7 sigma. The \(\gamma\)-ray observations of this SNR could be explained well either by a leptonic model or a hadronic model, in which a flat spectrum for the ejected electrons/protons.
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title Morphology Study for GeV Emission of the Nearby Supernova Remnant G332.5-5.6
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